Tarantula Nebula

The Tarantula Nebula was observed by Nicolas-Louis de Lacaille during an expedition to the Cape of Good Hope between 1751 and 1753.

[5] Johann Bode included the Tarantula in his 1801 Uranographia star atlas and listed it in the accompanying Allgemeine Beschreibung und Nachweisung der Gestirne catalog as number 30 in the constellation "Xiphias or Dorado".

[3] The nebula resides on the leading edge of the LMC where ram pressure stripping, and the compression of the interstellar medium likely resulting from this, is at a maximum.

[15] In addition to NGC 2070, the Tarantula Nebula contains several other star clusters including the much older Hodge 301.

[19] An x-ray quiet black hole was discovered in the Tarantula Nebula, the first outside of the Milky Way Galaxy that does not radiate strongly.

The brilliant stars in the Tarantula Nebula unleash a torrent of ultraviolet light and stellar winds that etch away at the hydrogen gas cloud in which the stars were born.
Hubble's high resolution view of the star-forming region of Tarantula Nebula and the R136 super star cluster at its center
Detail of RMC 136a , cluster NGC 2070
VFTS 243